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asteroseismicanalysisofacenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar
YanKe Tang1; ShaoLan Bi2; Ning Gai1; HuaYin Xu1
2008
Source Publicationchineseastronomyandastrophysics
ISSN0275-1062
Volume8Issue:4Pages:421
AbstractTaking into consideration the effects of rotation and interior magnetic field during the lifetime of the star, we reconstruct the model of a Cen B to satisfy the latest nonasteroseismic and asteroseismic observational constraints. We find that the effects can induce a change of about 0.3 μHz in the large frequency spacings and can speed up the star's evolution. The model of a Cen B has thereby been improved.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52234
Collection中国科学院国家天文台
Affiliation1.中国科学院国家天文台
2.北京师范大学
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
YanKe Tang,ShaoLan Bi,Ning Gai,et al. asteroseismicanalysisofacenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar[J]. chineseastronomyandastrophysics,2008,8(4):421.
APA YanKe Tang,ShaoLan Bi,Ning Gai,&HuaYin Xu.(2008).asteroseismicanalysisofacenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar.chineseastronomyandastrophysics,8(4),421.
MLA YanKe Tang,et al."asteroseismicanalysisofacenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar".chineseastronomyandastrophysics 8.4(2008):421.
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